The Interplay of Magnetic Fields, Turbulence and Vorticity in Core-Collapse Supernovae

arXiv:2608.24578 · astro-ph.SR, astro-ph.HE · Submitted 2026-08-25 · Read on arXiv

astro-ph.SR, astro-ph.HE

Submitted: 2026-08-25

Updated: 2026-08-25

Comments: Accepted for publication in Phys. Rev. D. 20 pages. 12 figures. Data behind figures available on zenodo

DOI: 10.1103/lgc5-tn23

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 53× in this paper · explained in 2 episodes
• Alignment — 11× in this paper · explained in 1 episode
• Accretion Shock — 6× in this paper · explained in 1 episode
• Metallicity — 4× in this paper · explained in 3 episodes
• Fidelity — 2× in this paper · explained in 2 episodes
• Local Spatial Average — 2× in this paper
• Conservation Laws — 1× in this paper · explained in 3 episodes
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes
• Texas Advanced Computing Center — 1× in this paper

Sources

• On the Nature of Core Collapse Supernova Explosions
• Long-Term Multidimensional Models of Core-Collapse Supernovae: Progress and Challenges
• Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
• Simulation of the Spherically Symmetric Stellar Core Collapse, Bounce, and Postbounce Evolution of a 13 Solar Mass Star with Boltzmann Neutrino Transport, and Its Implications for the Supernova Mechanism
• Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations
• Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature
• A Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Space-Time
• Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state
• Theory of Core-Collapse Supernovae
• Self-consistent 3D Supernova Models From -7 Minutes to +7 Seconds: a 1-bethe Explosion of a ~19 Solar-mass Progenitor
• Three-dimensional simulation of a core-collapse supernova for a binary star progenitor of SN 1987A
• The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis \`a vis One-Dimensional, Massive-star Supernova Progenitor Models
• Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields
• Three-dimensional GRMHD Simulations of Rapidly Rotating Stellar Core-Collapse
• Nucleosynthetic Analysis of Three-Dimensional Core-Collapse Supernova Simulations
• A Global Turbulence Model for Neutrino-Driven Convection in Core-Collapse Supernovae
• Hydrodynamics of Core-Collapse Supernovae at the Transition to Explosion. I. Spherical Symmetry
• Dimensional Dependence of the Hydrodynamics of Core-Collapse Supernovae
• Turbulence and magnetic field amplification from spiral SASI modes in core-collapse supernovae
• Toward connecting core-collapse supernova theory with observations: I. Shock revival in a 15 Msun blue supergiant progenitor with SN 1987A energetics

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